Image Details
 
                    Caption: Fig. 2.
Top panel: CMD of the Hyades sample with the mean polluted isochrone (solid line) and LOWESS fit (dashed line) superposed. Bottom panel: Scatter plot in Δ﹩M_{V}﹩ of the Hyades sample about the LOWESS fit. Superimposed are the differences between the 2 σ isochrones and the mean isochrone (dashed line: +2 σ; dotted line: −2 σ).
© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.